activity
19992005
most citedGetting Its Kicks: A VLBA Parallax for the Hyperfast Pulsar B1508+55

180 citations · 386 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph2005180 cited

Getting Its Kicks: A VLBA Parallax for the Hyperfast Pulsar B1508+55

S. Chatterjee, W. H. T. Vlemmings, W. F. Brisken +7

The highest velocity neutron stars establish stringent constraints on natal kicks, asymmetries in supernova core collapse, and the evolution of close binary systems. Here we presen…

astro-ph20051 cited

Pulsar Astrometry at the Microarcsecond Level

W. H. T. Vlemmings, S. Chatterjee, W. F. Brisken +12

Determination of pulsar parallaxes and proper motions addresses fundamental astrophysical questions. We have recently finished a VLBI astrometry project to determine the proper mot…

astro-ph2003139 cited

Pulsar Parallaxes at 5 GHz with the Very Long Baseline Array

S. Chatterjee, J. M. Cordes, W. H. T. Vlemmings +3

We present the first pulsar parallaxes measured with phase-referenced pulsar VLBI observations at 5 GHz. Due to the steep spectra of pulsars, previous astrometric measurements have…

astro-ph200366 cited

NE2001. II. Using Radio Propagation Data to Construct a Model for the Galactic Distribution of Free Electrons

J. M. Cordes, T. J. W. Lazio

In Paper I we present a new model for the Galactic distribution of free electrons. In this paper we describe the input data and methodology for determining the structure and parame…

astro-ph2001

Far-Infrared ISO Limits on Dust Disks around Millisecond Pulsars

T. J. W. Lazio, J. Fischer, R. S. Foster

We report 60 and 90 micron observations of 7 millisecond pulsars with the ISOPHOT instrument and describe our analysis procedures. No pulsars were detected, and typical (3σ) upper…

astro-ph1999

Discovery of a New Filamentary Structure near the Galactic Center: G358.85+0.47 - The Pelican

K. R. Anantharamaiah, C. C. Lang, N. E. Kassim +2

We report the discovery of a new filamentary structure, G358.85+0.47, consisting of at least three mutually parallel but bent `strands', located about 1.5 degrees SW of the Sgr A c…